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of having only #wo sources, we have nan. In this case, we would write the |
expression for 4A? as the sum of a whole lot of amplitudes, complex numbers, |
--- Trang 563 --- |
squared, and we would get the square of each one, all added together, plus cross |
terms bebween every pair, and if the cireumnstances are such that the latter average |
out, then there will be no effects ofinterference. It may be that the various sources |
are located in such random positions that, although the phase diference between |
4s and 4s is also defnite, it is very different from that bebtween 4: and 4a, etc. |
So we would get a whole lot of cosines, many plus, many minus, all averaging out. |
So it is that in many circumstances we do not see the efects of interference, |
but see only a collective, total intensity equal to the sum of all the intensities. |
32-5 Scattering of light |
The above leads us to an efect which occurs in air as a consequence of the |
Irregular positions of the atoms. When we were discussing the index of refraction, |
we saw that an incoming beam of light will make the atoms radiate again. The |
electric fñeld of the incoming beam drives the electrons up and down, and they |
radiate because of their acceleration. Phis scattered radiation combines to give |
a beam in the same direction as the incoming beam, but of somewhat diferent |
phase, and this is the origin of the index of refraction. |
But what can we say about the amount of re-radiated light in some other |
direction? Ordinarily, If the atoms are very beautifully located in a nice pattern, |
1t is easy to show that we get nothing in other directions, because we are adding |
a lot of vectors with their phases always changing, and the result comes to zero. |
But ïf the objects are randomlụ located, then the total intensity in any direction |
1s the sươn of the intensities that are scattered by each atom, as we have just |
discussed. Eurthermore, the atoms in a gas are in actual motion, so that although |
the relative phase of two atoms is a definite amount now, later the phase would be |
quite diferent, and therefore eøch cosine term will average out. Therefore, to fnd |
out how much light is scattered in a given direction by a gas, we merely study the |
efects of one øtom and multiply the intensity it radiates by the number of atoms. |
Barlier, we remarked that the phenomenon of scattering of light of this nature |
1s the origin of the blue of the sky. 'Phe sunlight goes through the air, and when |
we look to one side of the sun—say at 90° to the beam——we see blue light; what |
we now have to calculate is hou rmụch light we see and 0h it 1s blue. |
Tf the incident beam has the electric ñeld* E = oec”“f at the point where |
the atom is located, we know that an electron in the atom will vibrate up and |
- * When a Caret appears on a vector iÈ signifies that the componen‡s of the vector are complex: |
#2 = (E„y, lụ, E„). |
--- Trang 564 --- |
lncident beam + Atom |
(unpolarized) „ XS |
Scattered ¬ |
Fig. 32-2. A beam of radiation falls on an atom and causes the |
charges (electrons) in the atom to move. The moving electrons in turn |
radiate In varlous directions. |
down in response to this (Fig. 32-2). Erom Eq. (23.8), the response will be |
Ê=—> “—-: (32.15) |
m(uổ — 3 + iu) |
W© could include the damping and the possibility that the atom acts like several |
oscillators of diferent frequency and sum over the various frequencies, but for |
simplicity let us just take one oscillator and neglect the damping. Then the |
response to the external electric fñield, which we have already used in the calculation |
of the index of refraction, is simply |
&=—S—. (32.16) |
m(duỗ — œ3) |
We could now easily calculate the intensity of light that is emitted in various |
đirections, using formula (32.2) and the acceleration corresponding to the above Z. |
Rather than do this, however, we shall simply calculate the #ofal amownt oŸ |
light scattered in ai/ directions, just to save time. 'Phe total amount of light |
energy per second, scattered in all directions by the single atom, is oÝ course |
given by Eaq. (32.6). 5o, putting together the various pieces and regrouping them, |
W© getE |
P = [(q2ø*/12meoe))qễ Eỗ Jmà(Ÿ — œ8)” ] |
= (šeocE8)(8a/3)(q¿/16n2cm¿e")[j`/(ø2 — œ8)”] |
= (šcocE8)(Smr3/3)|°/(Ÿ — w)'] (32.17) |
for the total scattered power, radiated ín all directions. |
--- Trang 565 --- |
We have written the result in the above form because it is then easy %O |
remember: First, the total energy that is scattered is proportional to the square |
of the incident fñeld. What does that mean? Obviously, the square of the ineident |
field is proportional to the energy which is coming in per second. In fact, the |
energy incident per square meter per second is cọc times the average (H2) of |
the square of the electric field, and If lo is the maximum value of #, then |
(F2?) = šEÿ. In other words, the total energy scabtered is proportional to the |
energy per square meter that comes in; the brighter the sunlight that is shining |
in the sky, the brighter the sky is going to look. |
Next, what ƒfraction oŸ the incoming light is scattered? Let us imagine a |
“target” with a certain area, let us say ø, in the beam (not a real, material target, |
because this would difract light, and so on; we mean an imaginary area drawn |
in space). The total amount of energy that would pass through this surface ø |
in a given circumstance is proportional both to the incoming intensity and to ơ, |
and the total power would be |
P= (š‹ạcE))ø. (32.18) |
Now we invent an idea: we say that the atom scatters a total amount of |
intensity which is the amount which would fall on a certain geometrical area, |
and we give the answer by giving that area. That answer, then, is independent |
of the incident intensity; it gives the ratio of the energy scattered to the energy |
Ineident per square meter. In other words, the ratio |
total energy scattered per second : |
—————— san ørea. |
energy incident per square meter per second |
The signifcance of this area is that, if all the energy that impinged on that area |
were to be spewed in all directions, then that is the amount of energy that would |
be scattered by the atom. |
This area is called a cross seclion for scaftering; the idea OoŸ cross section 1s |
used constantly, whenever some phenomenon occurs in proportion to the intensity |
of a beam. In such cases one always describes the amount of the phenomenon by |
saying what the efective area would have to be to pick up that mụuch of the beam. |
lt does not mean in any way that this oscillator actually has such an area. If |
there were nothing present but a free electron shaking up and down there would |
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